基于地/空/月综合光学观测模型的地月空间目标精确定轨

IF 0.8 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS
Zhenqi Wang, Zhongmiao Sun, Bin Guan, Jianguo Yan, Shangbiao Sun, Wanling Yang, Jean-Pierre Barriot
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引用次数: 0

摘要

地月空间作为人类未来生存和发展的重要战略领域,已成为航天大国深空探索活动的新战场。在深空探测任务需求日益增长的推动下,对地月空间碎片的监测与预警日益成为当务之急。地月空间目标的精确定轨为碎片监测提供了必要的支持。在此背景下,本研究提出了一个地面/空间/月球综合光学观测模型,通过武汉大学行星大地测量团队自主开发的软件平台SPOT(小天体和行星精确定轨工具包)实现。我们对地月点L1、L4和L5的目标POD进行了数值模拟。结果表明,仅利用地面观测的定轨精度在几百米左右。天基观测可以作为地面数据的宝贵补充,在精度上有一定的提高。然而,月球观测的加入显著提高了定轨精度,将位置误差和不确定性降低到几十米的量级。此外,月球观测噪声水平的变化对轨道确定精度的影响比天基观测更大。最后,通过对比实验验证了求解太阳辐射压力系数Cr对提高定轨精度的必要性。这些发现突出了基于月球的光学观测在实现高精度地月空间目标轨道确定方面的巨大潜力,并为未来在深空态势感知和自主导航方面的进展提供了宝贵的见解。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Precise Orbit Determination for Cislunar Space Targets Based on Ground/Space/Lunar Based Integrated Optical Observation Model

Precise Orbit Determination for Cislunar Space Targets Based on Ground/Space/Lunar Based Integrated Optical Observation Model

Precise Orbit Determination for Cislunar Space Targets Based on Ground/Space/Lunar Based Integrated Optical Observation Model

Cislunar space, as a strategically significant domain for humanity’s future survival and development, has become a new battleground for deep space exploration activities among leading spacefaring nations. Driven by the growing demands for deep space exploration missions, the monitoring and early warning of cislunar space debris have increasingly become a priority. Precise orbit determination (POD) of cislunar space targets provides essential support for debris surveillance. Against this backdrop, this study proposes a ground/space/lunar integrated optical observation model, implemented through SPOT (Small Body and Planets Precise Orbit Determination Toolkit)—a software platform independently developed by Wuhan University’s Planetary Geodesy Team. We conducted numerical simulations for POD of targets at Earth–Moon libration points L1, L4, and L5. The results demonstrate that the orbit determination accuracy using only ground-based observations is on the order of several hundred meters. Space-based observations can serve as a valuable supplement to ground-based data, providing a modest improvement in accuracy. However, the addition of lunar-based observations significantly enhances the orbit determination accuracy, reducing position errors and uncertainties to the order of tens of meters. Furthermore, variations in the noise level of lunar-based observations have a stronger impact on orbit determination accuracy than space-based observations. Finally, comparative experiments verify the necessity of solving the solar radiation pressure coefficient Cr for improving orbit determination accuracy. These findings highlight the tremendous potential of lunar-based optical observations in achieving high-precision orbit determination for cislunar space targets and provide valuable insights for future advancements in deep-space situational awareness and autonomous navigation.

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来源期刊
Solar System Research
Solar System Research 地学天文-天文与天体物理
CiteScore
1.60
自引率
33.30%
发文量
32
审稿时长
6-12 weeks
期刊介绍: Solar System Research publishes articles concerning the bodies of the Solar System, i.e., planets and their satellites, asteroids, comets, meteoric substances, and cosmic dust. The articles consider physics, dynamics and composition of these bodies, and techniques of their exploration. The journal addresses the problems of comparative planetology, physics of the planetary atmospheres and interiors, cosmochemistry, as well as planetary plasma environment and heliosphere, specifically those related to solar-planetary interactions. Attention is paid to studies of exoplanets and complex problems of the origin and evolution of planetary systems including the solar system, based on the results of astronomical observations, laboratory studies of meteorites, relevant theoretical approaches and mathematical modeling. Alongside with the original results of experimental and theoretical studies, the journal publishes scientific reviews in the field of planetary exploration, and notes on observational results.
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